Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Ares Vallis: ESP_087933_1945 ESP_088645_1945 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.31 | 331. | 6.80 | -6.85 | 46.7 | 49.7 |
| Mounds in Oxia Colles: ESP_087801_2045 ESP_087735_2045 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.18 | 335. | -9.3 | 8.282 | 44.6 | 42.9 |
| Crater: ESP_087761_2120 ESP_087695_2120 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.74 | 346. | -8.7 | 7.579 | 43.4 | 41.8 |
| Layering in Southern Lucus Planum: ESP_087675_1680 ESP_086752_1680 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.0 | 178. | 8.97 | -14.1 | 59.4 | 52.3 |
| Crater in Arabia Terra: ESP_087747_2200 ESP_087681_2200 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.57 | 7.75 | -7.8 | 6.691 | 43.3 | 42.0 |
| Layering in Inverted Crater: ESP_087833_1725 ESP_088123_1725 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.44 | 186. | -19. | -2.53 | 59.3 | 59.4 |
| Crater Wall with Potential Chloride Deposit Outcrop: ESP_087806_1470 ESP_089164_1470 (Interval in Earth days: 106) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.8 | 205. | 3.46 | 14.06 | 74.8 | 74.9 |
| Fan or Delta Deposits in Northeast Hargraves Crater: ESP_087916_2010 ESP_087072_2010 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.98 | 75.9 | -5.5 | 6.04 | 45.3 | 41.6 |
| Terrain Northeast of Pollack Crater: ESP_087786_1735 ESP_088498_1735 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.28 | 27.9 | 3.19 | -8.79 | 56.9 | 59.9 |
| Dark Material in Coprates Chasma: ESP_087697_1660 ESP_088198_1660 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.7 | 298. | 0.73 | 12.47 | 61.2 | 62.7 |
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